A molecular line survey toward the nearby galaxies NGC 1068, NGC 253, and IC 342 at 3 mm with the Nobeyama 45 m radio telescope: Impact of an AGN on 1 kpc scale molecular abundances-Reference-Cited by-同舟云学术

A molecular line survey toward the nearby galaxies NGC 1068, NGC 253, and IC 342 at 3 mm with the Nobeyama 45 m radio telescope: Impact of an AGN on 1 kpc scale molecular abundances

Published:2018-01-01 Issue:1 Volume:70 Page:
ISSN:0004-6264
Container-title:Publications of the Astronomical Society of Japan
language:en
Short-container-title:

Author:

Nakajima Taku¹,Takano Shuro²³,Kohno Kotaro⁴⁵,Harada Nanase⁶,Herbst Eric⁷

Affiliation:

1. Institute for Space-Earth Environmental Research, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi 464-8601, Japan

2. Nobeyama Radio Observatory, National Astronomical Observatory of Japan, 462-2 Nobeyama, Minamimaki, Minamisaku, Nagano 384-1305, Japan

3. Department of Astronomical Science, The Graduate University for Advanced Studies (SOKENDAI), 462-2 Nobeyama, Minamimaki, Minamisaku, Nagano 384-1305, Japan

4. Institute of Astronomy, The University of Tokyo, 2-21-1, Osawa, Mitaka, Tokyo 181-0015, Japan

5. Research Center for Early Universe, School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan

6. Academia Sinica Institute of Astronomy and Astrophysics, P.O. Box 23-141, Taipei 10617, Taiwan

7. Department of Chemistry, University of Virginia, McCormick Road, P.O. Box 400319, Charlottesville, VA 22904, USA

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/pasj/article-pdf/70/1/7/24001208/psx153.pdf

Reference143 articles.

1. CN and HNC line emission in IR luminous galaxies

2. Aλ = 3 mm molecular line survey of NGC 1068

3. Lambda = 3 mm line survey of nearby active galaxies

4. Aλ= 1.3 mm and 2 mm molecular line survey towards M 82

5. CS, HC3N, and CH3CCH multi-line analyses toward starburst galaxies

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